Abstract The analysis presented shows that the classical model of non-linear magnetic field line reconnection changes considerably in the presence of sheared magnetic fields and/or high tangential plasma flow components. This shear excites large amplitude Alfvén waves on both sides of the reconnection layer where the magnetic field is rotated to a common direction within the layer. In addition two slow shock (or rarefaction) waves within the reconnection layer are necessary to account for the remaining shear in plasma flow. The detailed structures of such reconnection layers with implications for magnetopause reconnection events are discussed.
Reconnection active layers
Advances in Space Research ; 6 , 1 ; 119-121
1986-01-01
3 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Train reconnection control circuit and method and reconnection train
Europäisches Patentamt | 2023
|Tema Archiv | 1986
|British Library Conference Proceedings | 2002
|Online Contents | 2002
|Magnetic Fluxtube Reconnection
British Library Conference Proceedings | 1997
|